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Outer Van Allen Radiation Belt Response to Interacting Interplanetary Coronal Mass Ejections
dc.contributor.authorKilpua, E. K. J.
dc.contributor.authorTurner, D. L.
dc.contributor.authorJaynes, A. N.
dc.contributor.authorHietala, H.
dc.contributor.authorKoskinen, H. E. J.
dc.contributor.authorOsmane, A.
dc.contributor.authorPalmroth, M.
dc.contributor.authorPulkkinen, T. I.
dc.contributor.authorVainio, R.
dc.contributor.authorBaker, D.
dc.contributor.authorClaudepierre, S. G.
dc.date.accessioned2019-05-31T18:26:54Z
dc.date.available2020-05-01T18:03:25Zen
dc.date.issued2019-03
dc.identifier.citationKilpua, E. K. J.; Turner, D. L.; Jaynes, A. N.; Hietala, H.; Koskinen, H. E. J.; Osmane, A.; Palmroth, M.; Pulkkinen, T. I.; Vainio, R.; Baker, D.; Claudepierre, S. G. (2019). "Outer Van Allen Radiation Belt Response to Interacting Interplanetary Coronal Mass Ejections." Journal of Geophysical Research: Space Physics 124(3): 1927-1947.
dc.identifier.issn2169-9380
dc.identifier.issn2169-9402
dc.identifier.urihttps://hdl.handle.net/2027.42/149291
dc.description.abstractWe study the response of the outer Van Allen radiation belt during an intense magnetic storm on 15–22 February 2014. Four interplanetary coronal mass ejections (ICMEs) arrived at Earth, of which the three last ones were interacting. Using data from the Van Allen Probes, we report the first detailed investigation of electron fluxes from source (tens of kiloelectron volts) to core (megaelectron volts) energies and possible loss and acceleration mechanisms as a response to substructures (shock, sheath and ejecta, and regions of shock‐compressed ejecta) in multiple interacting ICMEs. After an initial enhancement induced by a shock compression of the magnetosphere, core fluxes strongly depleted and stayed low for 4 days. This sustained depletion can be related to a sequence of ICME substructures and their conditions that influenced the Earth’s magnetosphere. In particular, the main depletions occurred during a high‐dynamic pressure sheath and shock‐compressed southward ejecta fields. These structures compressed/eroded the magnetopause close to geostationary orbit and induced intense and diverse wave activity in the inner magnetosphere (ULF Pc5, electromagnetic ion cyclotron, and hiss) facilitating both effective magnetopause shadowing and precipitation losses. Seed and source electrons in turn experienced stronger variations throughout the studied interval. The core fluxes recovered during the last ICME that made a glancing blow to Earth. This period was characterized by a concurrent lack of losses and sustained acceleration by chorus and Pc5 waves. Our study highlights that the seemingly complex behavior of the outer belt during interacting ICMEs can be understood by the knowledge of electron dynamics during different substructures.Key PointsDetailed response of the outer belt to substructures in a complex solar wind driver is investigatedMost substructures in the interacting ICMEs here deplete the core radiation belt population but inject source electronsCore electrons were enhanced during sustained chorus and Pc5 activity and lack of losses
dc.publisherWiley Periodicals, Inc.
dc.publisherAmerican Geophysical Union
dc.subject.otherinterplanetary coronal mass ejections
dc.subject.otherradiation belts
dc.subject.otherouter belt
dc.subject.othersolar wind
dc.subject.othermagnetospheric waves
dc.subject.othermagnetospheric storm
dc.titleOuter Van Allen Radiation Belt Response to Interacting Interplanetary Coronal Mass Ejections
dc.typeArticle
dc.rights.robotsIndexNoFollow
dc.subject.hlbsecondlevelAstronomy and Astrophysics
dc.subject.hlbtoplevelScience
dc.description.peerreviewedPeer Reviewed
dc.description.bitstreamurlhttps://deepblue.lib.umich.edu/bitstream/2027.42/149291/1/jgra54856_am.pdf
dc.description.bitstreamurlhttps://deepblue.lib.umich.edu/bitstream/2027.42/149291/2/jgra54856.pdf
dc.identifier.doi10.1029/2018JA026238
dc.identifier.sourceJournal of Geophysical Research: Space Physics
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